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• W2064923241 abstract "To investigate the possible cooling of the corona by soft X-rays bursts, we have studied 114 bursts embedded in the known X-ray evolution of 4U 1636−536. We have grouped these bursts according to the ratio of the flux in the 1.5–12 keV band with respect to that in the 15–50 keV band, as monitored by Rossi X-ray Timing Explorer/All Sky Monitor and Swift/Burst Alert Telescope, respectively. We have detected a shortage at hard X-rays while bursting. This provides hints for a corona cooling process driven by soft X-rays fed by the bursts that occurred on the surface of neutron star. The flux shortage at 30–50 keV has a time lag of 2.4 ± 1.5 s with respect to that at 2–10 keV, which is comparable to that of 0.7 ± 0.5 s reported in bursts of IGR 17473−2721. We comment on the possible origin of these phenomena and on the implications for the models on the location of the corona." @default.
• W2064923241 created "2016-06-24" @default.
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• W2064923241 date "2013-05-09" @default.
• W2064923241 modified "2023-09-30" @default.
• W2064923241 title "X-ray bursts as a probe of the corona: the case of XRB 4U 1636−536" @default.
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• W2064923241 doi "https://doi.org/10.1093/mnras/stt625" @default.
• W2064923241 hasPublicationYear "2013" @default.
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